SST/SAGE and HST Study of Stellar Populations and Star Formation around NGC 1850 in the LMC

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

Combining the high angular resolution (< 0.1") and deep HST optical images of limited area fields with the SAGE survey observations of the LMC obtained in the NIR/MIR with Spitzer at lower angular resolution (> 1") but with deep exposures, allows one to reach an excellent understanding of the processes governing the formation of moderate to low mass stars (0.8-2 MSun), which represent the bulk of the stellar mass in galaxies. We have followed this approach to study the properties of the young populations present in the region around the double cluster NGC 1850 and their relationsip with both the diffuse medium and the older stellar populations.

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